And finally the location of meteor echoes after calibration is found.
并用校正后的数据来计算流星回波的空间位置。
The torque is measured, and can be converted to apparent viscosity after calibration.
旋矩是可以测量的，在校正后并可转换成可见的粘度。
The real question is how bright the picture is after calibration for ideal cinema viewing.
真正的问题是多么的光明图片是校准后的理想电影院观看。
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